Open Access

Fig. 6.

image

Stellar mass as a function of redshift for the parent sample of 2483 galaxies drawn from MUSE deep observations in HUDF (gray dots), HDFS (blue dots), A2744 (red dots), and CGR30 (green dots). Thanks to the high sensitivity of MUSE, star-forming galaxies are identified with a secure spectroscopic redshift up to z ∼ 6 over a large range of stellar masses (∼ 107 − 1011 M), except in the so-called “redshift desert” (z ∼ 1.5−2.8) where galaxies in the low-mass regime (M ∼ 107 − 108M) are detected behind the A2744 lensing cluster only.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.